Cosmological Models with Some Interacting Physical Distribution
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Cosmological Models with Some Interacting Physical Distribution (Paperback) (2015)
DE PB NW RPISBN: 9783659744365 bzw. 3659744360, in Deutsch, LAP Lambert Academic Publishing, United States, Taschenbuch, neu, Nachdruck.
Von Händler/Antiquariat, The Book Depository EURO [60485773], London, United Kingdom.
Language: English . Brand New Book ***** Print on Demand *****.Einstein s discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist.
Language: English . Brand New Book ***** Print on Demand *****.Einstein s discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist.
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Cosmological Models with Some Interacting Physical Distribution | A Study of Inflationary Universe | | Taschenbuch | Paperback | 136 S. | Englisch | 2015 | EAN 9783659744365 (2015)
~EN PB NWISBN: 9783659744365 bzw. 3659744360, vermutlich in Englisch, 136 Seiten, LAP LAMBERT Academic Publishing, Taschenbuch, neu.
Lieferung aus: Deutschland, Versandkosten nach: Deutschland, Versandkostenfrei.
Von Händler/Antiquariat, preigu, [5789586].
Einstein¿s discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the... 2015, Taschenbuch, Neuware, 221g, 136, Banküberweisung, PayPal, Klarna-Sofortüberweisung.
Von Händler/Antiquariat, preigu, [5789586].
Einstein¿s discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the... 2015, Taschenbuch, Neuware, 221g, 136, Banküberweisung, PayPal, Klarna-Sofortüberweisung.
3
Cosmological Models with Some Interacting Physical Distribution (2015)
~EN PB NWISBN: 9783659744365 bzw. 3659744360, vermutlich in Englisch, LAP LAMBERT Academic Publishing, Taschenbuch, neu.
Lieferung aus: Deutschland, Lieferbar in 2 - 3 Tage.
Einstein's discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist. Taschenbuch, 11.07.2015.
Einstein's discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist. Taschenbuch, 11.07.2015.
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Cosmological Models with Some Interacting Physical Distribution
~EN NW ABISBN: 9783659744365 bzw. 3659744360, vermutlich in Englisch, neu, Hörbuch.
Lieferung aus: Schweiz, Lieferzeit: 2 Tage, zzgl. Versandkosten.
Einstein's discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist.
Einstein's discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist.
5
Cosmological Models with Some Interacting Physical Distribution - A Study of Inflationary Universe
DE PB NWISBN: 9783659744365 bzw. 3659744360, in Deutsch, LAP Lambert Academic Publishing, Taschenbuch, neu.
Lieferung aus: Deutschland, Versandkostenfrei.
Cosmological Models with Some Interacting Physical Distribution: Einstein`s discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist. Englisch, Taschenbuch.
Cosmological Models with Some Interacting Physical Distribution: Einstein`s discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist. Englisch, Taschenbuch.
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Cosmological Models with Some Interacting Physical Distribution (2015)
EN PB USISBN: 9783659744365 bzw. 3659744360, in Englisch, 136 Seiten, LAP Lambert Academic Publishing, Taschenbuch, gebraucht.
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Von Händler/Antiquariat, super_star_seller.
Einstein's discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist. Paperback, Label: LAP Lambert Academic Publishing, LAP Lambert Academic Publishing, Produktgruppe: Book, Publiziert: 2015-06-16, Studio: LAP Lambert Academic Publishing.
Von Händler/Antiquariat, super_star_seller.
Einstein's discovery of general relativity in the last century enabled us for the first time in history to come up with a compelling, testable theory of the Universe. There are two aspects of cosmology. First, there is an enormous amount of data today. The other aspect of modern cosmology is that we have developed a consistent theoretical framework which agrees quantitatively with data. These two features are the secret of the modern cosmology. The realisation that the Universe is expanding and was once much hotter and denser, can be tested against astronomical data. The theoretical and observational developments in the last two decades of the 20th century point to the existence of dark matter and dark energy, the evolution of perturbations around the zero order smooth Universe and inflation. This book mainly concentrates on the physical and large scale geometrical aspects of expanding Universe which is consistent with the present observations of the Universe. It mainly describe the physical and geometrical properties of the cosmological models when physical distributions like zero-mass scalar field, scalar field, bulk viscosity and dynamic dark energy density exist. Paperback, Label: LAP Lambert Academic Publishing, LAP Lambert Academic Publishing, Produktgruppe: Book, Publiziert: 2015-06-16, Studio: LAP Lambert Academic Publishing.
8
Cosmological Models with Some Interacting Physical Distribution
~EN PB NWISBN: 3659744360 bzw. 9783659744365, vermutlich in Englisch, LAP Lambert Academic Publishing, Taschenbuch, neu.
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